An infrared nebula in the Chamaeleon T association

Details An infrared nebula in the Chamaeleon T association An infrared nebula in the Chamaeleon T association

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aj.....88.1665s&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 88, Nov. 1983, p. 1665-1669.

Astronomy and Astrophysics

Astronomy

27

Astronomical Photography, Electrophotometry, Infrared Stars, Nebulae, Cosmic Dust, Emission Spectra, Interstellar Gas, Schmidt Telescopes, Spectral Energy Distribution, Ubv Spectra

Scientific paper

Data are tabulated for seven nebulae in the Chamaeleon T association. Three, which are large and clearly related to illuminating stars, appear to be typical reflection nebulae. Three are small wisps attached to stars and are probably cometary-type reflection nebulae. The remaining nebula is a triangular wisp having an unusually red spectral energy distribution and showing no illuminating star on visual wavelength photographs. The western tip of this nebula coincides closely with the position of a recently reported infrared source. The nebula is probably one lobe of a bipolar nebula.

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